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英語人>網(wǎng)絡(luò)例句>ionosphere 相關(guān)的網(wǎng)絡(luò)例句
ionosphere相關(guān)的網(wǎng)絡(luò)例句

查詢詞典 ionosphere

與 ionosphere 相關(guān)的網(wǎng)絡(luò)例句 [注:此內(nèi)容來源于網(wǎng)絡(luò)人人操又人人,僅供參考]

It is also found that the ionosphere manifests the asymmetry in response to north- and southward horizontal winds and to day and night winds, and also shows latitudinal difference.

對電離層峰值高度響應(yīng)水平中性風(fēng)的數(shù)值計(jì)算表明,響應(yīng)存在著對南北方向風(fēng)的不對稱性一级特黄性色生活片一区二区、日夜不對稱性和緯度差異av大陆老熟女性爱。

Can be used to describe the ionosphere and the magnetosphere of the electromagnetic field disturbance.

可用來描述電離層和磁層的電磁場擾動(dòng)女人与拘性行为视频网站。

In midlatitude, the ionospheric response to southward turnings in summer and equinox and by night is stronger, which fades out with latitude decreases. During the recovery phase the irregular fluctuation in the ionosphere comes forth. In low-latitude, the disturbance caused by the turnings is strong in summer and equinox and weak in winter, although it tends to be immersing into the background disturbances.

在中緯啊啊啊啊啊啊网站,發(fā)生在夏分季和夜間的翻轉(zhuǎn)能造成較強(qiáng)的電離層負(fù)響應(yīng)成年黄页网站免费观看视频,其幅度隨緯度的降低而變?nèi)跞张產v网,在恢?fù)過程中存在不規(guī)則振蕩;在低緯一级片视频久久手机导航,南向翻轉(zhuǎn)引起的電離層響應(yīng)在夏分季較強(qiáng)色色色视频免费网址,在冬季則較弱,且易被淹沒在電離層自身的擾動(dòng)中成人小蝌蚪视频破解网站。

By measuring the instantaneous value of short-wave spectrum, we can get an important parameter of the local ionosphere, foF2, and then work out the MUF of the electrocircuit.

通過對測試結(jié)果進(jìn)行統(tǒng)計(jì)分析可以得出:短波頻譜的一階矩ICF和電離層F2層臨界頻率f0F2具有很好的相關(guān)特性,通過測量短波頻譜的瞬時(shí)值可以得到本地電離層的重要參量f0F2一级二级性爱视频,進(jìn)而可以計(jì)算出電路的最高可用頻率97视频免费在线。

The ability of the ionosphere to reflect these waves is dependent upon normal variations in the electron density at different levels.

電離層反射電波的能力取決于不同高度上電子密度的正常差別。

GPS radio occultation measurements are brand-new and highly effective, which can detect atmosphere and ionosphere, but still in the development and perfection.

GPS無線電掩星技術(shù)是嶄新的在线不卡精品、高效的地球大氣層和電離層探測技術(shù)哟色网站,但仍在發(fā)展和完善之中。

On the basis of setting up a model of the parallel transmission link of short-wave data communication system, this paper analyses the anti-noise performance of data communication in a non-selective Rayleigh gradually fading ionosphere channel, and derives the average error code rate formular and its curves.

在建立并發(fā)制短波數(shù)據(jù)通信系統(tǒng)模型的基礎(chǔ)上人人操人人干com,分析了非選擇性瑞利慢衰落電離層信道中數(shù)據(jù)通信抗噪聲性能免费在线观看黄色级视频,并導(dǎo)出了平均誤碼率公式,生成了誤碼率曲線色影库,為雷達(dá)情報(bào)短波數(shù)據(jù)通信鏈路的仿真及效能評估提供理論依據(jù)

In this approach, double-differenced dual-frequency phase measurements and the known coordinates of reference stations as well as the precise ephemeris are used to rebuild observation equation, and then a Kalman filter is designed for the parameters estimation, i.e. ionosphere delay etc.

該算法使用雙差雙頻相位久久免费看黄A级毛片美国、參考站精確的坐標(biāo)和精密星歷構(gòu)造觀測量,并用卡爾曼濾波來估計(jì)電離層參數(shù)欧美第1页,在給定顯著水平的情況下美女脱光黄色网站,可以使用單個(gè)或少量歷元以假設(shè)檢驗(yàn)的方法探測和修復(fù)周跳。

In our views, the region of the CMI, near the ionosphere of Saturn (1 Saturn radius above the polar area), is regarded as the same area as the Saturn's Kilometric Radiation Source.In this paper, we deduce that the KHI will appear before 11 LT (Saturn's Local Time), the Alfven wave will take 383 min to reach Saturn, the sunward magnetic line will bend almost 80°. Finally, we get the distribution of SKR source. It locates from 7~9 LT at a relatively lower latitude to 18 LT at the eveningside.

本文求出了磁層頂附近開爾文-亥姆霍茲不穩(wěn)定性發(fā)生在土星本地時(shí)(Saturn's Local Time)11 LT以前欧美日韩一区综合,得出了阿爾芬波沿磁力線傳播到土星需要約383 min国产在线精品26uuu,求解出向陽面磁力線彎曲了約80°,最后得出土星千米波輻射源分布從黎明段的7~9 LT延伸到傍晚段的18 LT一级婬片A片AAA毛片,并且黎明段分布的緯度比傍晚段低av片在线免费的。

In our views, the region of the CMI, near the ionosphere of Saturn (1 Saturn radius above the polar area), is regarded as the same area as the Saturn's Kilometric Radiation Source. In this paper, we deduce that the Kill will appear before 11 LT (Saturn's Local Time), the Alfven wave will take 38.3min to reach Saturn, the sunward magnetic line will bend almost 80°. Finally, we get the distribution of SKR source. It locates from 7~9 LT at a relatively lower latitude to 18 LT at the eveningside.

本文求出了磁層頂附近開爾文-亥姆霍茲不穩(wěn)定性發(fā)生在土星本地時(shí)(Satrun's Local Time)11LT以前,得出了阿爾芬波沿磁力線傳播到土星需要約38.3min欧美在线这里只有精品,求解出向陽面磁力線彎曲了約80°国产淫秽,最后得出土星千米波輻射源分布從黎明段的7~9LT延伸到傍晚段的18LT,并且黎明段分布的緯度比傍晚段低www色色。

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